Star-forming galaxies at cosmic noon

NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

Modeling the panchromatic spectral energy distributions of galaxies

C Conroy - Annual Review of Astronomy and Astrophysics, 2013 - annualreviews.org
The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

CEERS Epoch 1 NIRCam imaging: reduction methods and simulations enabling early JWST science results

MB Bagley, SL Finkelstein… - The Astrophysical …, 2023 - iopscience.iop.org
We present the data release and data reduction process for the Epoch 1 NIRCam
observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data …

JADES initial data release for the Hubble Ultra Deep Field: revealing the faint infrared sky with deep JWST NIRCam imaging

MJ Rieke, B Robertson, S Tacchella… - The Astrophysical …, 2023 - iopscience.iop.org
JWST has revolutionized the field of extragalactic astronomy with its sensitive and high-
resolution infrared view of the distant Universe. Adding to the new legacy of JWST …

Inferring the star formation histories of massive quiescent galaxies with bagpipes: evidence for multiple quenching mechanisms

AC Carnall, RJ McLure, JS Dunlop… - Monthly Notices of the …, 2018 - academic.oup.com
ABSTRACT We present Bayesian Analysis of Galaxies for Physical Inference and Parameter
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …

A Census of the Bright z= 8.5–11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields

SL Finkelstein, M Bagley, M Song… - The Astrophysical …, 2022 - iopscience.iop.org
We present the results from a new search for candidate galaxies at z≈ 8.5–11 discovered
over the 850 arcmin 2 area probed by the Cosmic Assembly Near-Infrared Deep …

The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for∼ 100,000 galaxies

IG Momcheva, GB Brammer… - The Astrophysical …, 2016 - iopscience.iop.org
We present reduced data and data products from the 3D-HST survey, a 248-orbit HST
Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five …

The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics

M Donnari, A Pillepich, D Nelson… - Monthly Notices of …, 2019 - academic.oup.com
We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …

The Herschel view of the dominant mode of galaxy growth from z= 4 to the present day

C Schreiber, M Pannella, D Elbaz, M Béthermin… - Astronomy & …, 2015 - aanda.org
We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

3D-HST+ CANDELS: the evolution of the galaxy size–mass distribution since z= 3

A van der Wel, M Franx, PG Van Dokkum… - The Astrophysical …, 2014 - iopscience.iop.org
Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …